A relational quantum field theory for scalars is built from Poincaré-covariant quantum reference frames, yielding local observables and fields that satisfy causality and reproduce key Wightman and Algebraic QFT properties.
Algebraic quantum field theory in curved spacetimes
2 Pith papers cite this work. Polarity classification is still indexing.
abstract
This article sets out the framework of algebraic quantum field theory in curved spacetimes, based on the idea of local covariance. In this framework, a quantum field theory is modelled by a functor from a category of spacetimes to a category of ($C^*$)-algebras obeying supplementary conditions. Among other things: (a) the key idea of relative Cauchy evolution is described in detail, and related to the stress-energy tensor; (b) a systematic "rigidity argument" is used to generalise results from flat to curved spacetimes; (c) a detailed discussion of the issue of selection of physical states is given, linking notions of stability at microscopic, mesoscopic and macroscopic scales; (d) the notion of subtheories and global gauge transformations are formalised; (e) it is shown that the general framework excludes the possibility of there being a single preferred state in each spacetime, if the choice of states is local and covariant. Many of the ideas are illustrated by the example of the free Klein-Gordon theory, which is given a new "universal definition".
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Back-action from Unruh-DeWitt detectors produces energy fluxes that exactly account for detector transitions due to the Unruh effect, including negative energy density regions near the Rindler horizon and in the far future for ground-state accelerated detectors.
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Foundations of Relational Quantum Field Theory I: Scalars
A relational quantum field theory for scalars is built from Poincaré-covariant quantum reference frames, yielding local observables and fields that satisfy causality and reproduce key Wightman and Algebraic QFT properties.
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Back-action from inertial and non-inertial Unruh-DeWitt detectors revisited in covariant perturbation theory
Back-action from Unruh-DeWitt detectors produces energy fluxes that exactly account for detector transitions due to the Unruh effect, including negative energy density regions near the Rindler horizon and in the far future for ground-state accelerated detectors.